20 Planetology07aaa0
... 6. <10% of the mass accretes into larger and larger particles which eventually form planetesimals (60 – 100). As the planetesimals collided, they grew in size and mass (gravitational attraction), but fewer in number, to form the planets. Large collisions among planetesimals resulted in: a) b) ...
... 6. <10% of the mass accretes into larger and larger particles which eventually form planetesimals (60 – 100). As the planetesimals collided, they grew in size and mass (gravitational attraction), but fewer in number, to form the planets. Large collisions among planetesimals resulted in: a) b) ...
Chart_set_4
... Some clumps within clouds collapse under their own weight to form stars or clusters of stars. Clumps spin at about 1 km/s. ...
... Some clumps within clouds collapse under their own weight to form stars or clusters of stars. Clumps spin at about 1 km/s. ...
Physics of the solar system10 Jan Announcements • Phenomena in the solar system and the
... driving me around, while I was considering again and again… that my apparent triumph over Mars has been in vain, I stumbled entirely by chance on the secant of the angle 5 18’, which is the measure of the greatest optical elongation. When I realized that this secant equals 1.00429, I felt ...
... driving me around, while I was considering again and again… that my apparent triumph over Mars has been in vain, I stumbled entirely by chance on the secant of the angle 5 18’, which is the measure of the greatest optical elongation. When I realized that this secant equals 1.00429, I felt ...
The Nine Planets
... Highly elliptical orbit - in about 290 years, Eris will move close enough to the Sun to partially thaw & melt away. Named after the Greek goddess of conflict ...
... Highly elliptical orbit - in about 290 years, Eris will move close enough to the Sun to partially thaw & melt away. Named after the Greek goddess of conflict ...
Unit 3: Understanding the Universe
... Enduring Understandings The solar system contains planets, dwarf planets, comets, asteroids, and other small solar system bodies. ...
... Enduring Understandings The solar system contains planets, dwarf planets, comets, asteroids, and other small solar system bodies. ...
Solar System research questions Group 1 River, Mark, Tommy
... Research Jupiter’s story of formation – how it wandered through the solar system and the consequences of that. Some of the large planets have sets of moons in retrograde revolutions around the planet. Which planets? How could that be explained? Why is Uranus orbiting on its side? Why don’t its rings ...
... Research Jupiter’s story of formation – how it wandered through the solar system and the consequences of that. Some of the large planets have sets of moons in retrograde revolutions around the planet. Which planets? How could that be explained? Why is Uranus orbiting on its side? Why don’t its rings ...
U 7 Synopsis
... and ice joined together chemically or as a result of collisions or electric forces of various kinds to form larger lumps, a bit like comets or asteroids. Eventually, within each orbit more and more lumps combined to form huge ‘planetesimals’, until in most orbits all the matter was absorbed within a ...
... and ice joined together chemically or as a result of collisions or electric forces of various kinds to form larger lumps, a bit like comets or asteroids. Eventually, within each orbit more and more lumps combined to form huge ‘planetesimals’, until in most orbits all the matter was absorbed within a ...
.SOL 4.7 Earth Patterns, Cycles, and Change Question/Answer Packet
... Jupiter-Watermelon, Saturn-large grapefruit, Uranus-apple, Neptune-lime, Venus-cherry tomato, Earth-cherry tomato, Mars-blueberry, Mercury-peppercorn ...
... Jupiter-Watermelon, Saturn-large grapefruit, Uranus-apple, Neptune-lime, Venus-cherry tomato, Earth-cherry tomato, Mars-blueberry, Mercury-peppercorn ...
Constructing a Solar System
... Solar systems form from swirling clouds of material where the massive center has a star form. The cloud would look somewhat like a hurricane. This is an image of Ivan in 2004 (from NOAA) in the Gulf of Mexico. What direction is it rotating – CW (clockwise) or CCW (counter-clockwise)? ...
... Solar systems form from swirling clouds of material where the massive center has a star form. The cloud would look somewhat like a hurricane. This is an image of Ivan in 2004 (from NOAA) in the Gulf of Mexico. What direction is it rotating – CW (clockwise) or CCW (counter-clockwise)? ...
Star Systems FINAL EXAM STUDY GUIDE
... -You should be able to recognize photographs of the major planets and the moons listed above taken from telescopes, satellite or probe images, or images from the surface. -Even though you wont be asked to identify images of them, you should know the names of Uranus’ and Pluto’s major Moons, as well ...
... -You should be able to recognize photographs of the major planets and the moons listed above taken from telescopes, satellite or probe images, or images from the surface. -Even though you wont be asked to identify images of them, you should know the names of Uranus’ and Pluto’s major Moons, as well ...
Instruction for making planet booklet
... This book has been designed to be printed out double sided, but you can make two separate booklets, one of the rock planets and one of the gas planets. For the double sided booklet, Select page 2,3 and print double sided. ...
... This book has been designed to be printed out double sided, but you can make two separate booklets, one of the rock planets and one of the gas planets. For the double sided booklet, Select page 2,3 and print double sided. ...
Planetary Mnemonic
... planets, one dwarf planet, their moons, and smaller objects (comets, asteroids, and meteoroids). The planets, moons, and smaller objects are held in orbit by the Sun's gravity. The sun is the only star in our solar system. Even though it's just an average-sized star, the Sun is still bigger and more ...
... planets, one dwarf planet, their moons, and smaller objects (comets, asteroids, and meteoroids). The planets, moons, and smaller objects are held in orbit by the Sun's gravity. The sun is the only star in our solar system. Even though it's just an average-sized star, the Sun is still bigger and more ...
etlife_exoplanets - University of Glasgow
... We can use spectral lines, like fingerprints, to identify the chemicals that stars and planets are made of. ...
... We can use spectral lines, like fingerprints, to identify the chemicals that stars and planets are made of. ...
Lecture 13
... • It would take 2000x the whole world’s energy output to propel a spaceship to half of the speed of light ...
... • It would take 2000x the whole world’s energy output to propel a spaceship to half of the speed of light ...
The formation of the Solar System I. Stellar context
... Sun contains 99.9% of Solar System's mass. Inner planets rocky, outer planets/satellites icy or heavily gas-rich Very similar isotopic ratios of certain elements ...
... Sun contains 99.9% of Solar System's mass. Inner planets rocky, outer planets/satellites icy or heavily gas-rich Very similar isotopic ratios of certain elements ...
ppt
... similar to a class of asteroid Matches mixture of organic compounds from carbonaceous meteorites, ice and hydrated silicates ...
... similar to a class of asteroid Matches mixture of organic compounds from carbonaceous meteorites, ice and hydrated silicates ...
Questions to answer - high school teachers at CERN
... R* is the rate of star formation in our galaxy fp is the fraction of those stars that have planets ne is average number of planets that can potentially support life per star fl is the fraction of the above that actually go on to develop life fi is the fraction of the above that actually go on to dev ...
... R* is the rate of star formation in our galaxy fp is the fraction of those stars that have planets ne is average number of planets that can potentially support life per star fl is the fraction of the above that actually go on to develop life fi is the fraction of the above that actually go on to dev ...
17.Extra-solar
... As a planet revolves around its star, it pulls the star around through its orbit. If the system is oriented face-on and the orbiting planet is massive enough, this small motion of the star can be detected by astrometry. As the planet moves through its orbit (red dots), the star revolves around the s ...
... As a planet revolves around its star, it pulls the star around through its orbit. If the system is oriented face-on and the orbiting planet is massive enough, this small motion of the star can be detected by astrometry. As the planet moves through its orbit (red dots), the star revolves around the s ...
File
... similarities between the planets, moons, asteroids and comets, we can gain a fuller understanding of the solar system as a whole. ...
... similarities between the planets, moons, asteroids and comets, we can gain a fuller understanding of the solar system as a whole. ...
Chapter 7 Our Planetary System What does the solar system look
... •! Many moons, including cloudy Titan ...
... •! Many moons, including cloudy Titan ...
Dwarf planet
A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite. That is, it is in direct orbit of the Sun, and is massive enough for its shape to be in hydrostatic equilibrium under its own gravity, but has not cleared the neighborhood around its orbit.The term dwarf planet was adopted in 2006 as part of a three-way categorization of bodies orbiting the Sun, brought about by an increase in discoveries of objects farther away from the Sun than Neptune that rivaled Pluto in size, and finally precipitated by the discovery of an even more massive object, Eris. The exclusion of dwarf planets from the roster of planets by the IAU has been both praised and criticized; it was said to be the ""right decision"" by astronomer Mike Brown, who discovered Eris and other new dwarf planets, but has been rejected by Alan Stern, who had coined the term dwarf planet in 1990.The International Astronomical Union (IAU) currently recognizes five dwarf planets: Ceres, Pluto, Haumea, Makemake, and Eris. Brown criticizes this official recognition: ""A reasonable person might think that this means that there are five known objects in the solar system which fit the IAU definition of dwarf planet, but this reasonable person would be nowhere close to correct.""It is suspected that another hundred or so known objects in the Solar System are dwarf planets. Estimates are that up to 200 dwarf planets may be found when the entire region known as the Kuiper belt is explored, and that the number may exceed 10,000 when objects scattered outside the Kuiper belt are considered. Individual astronomers recognize several of these, and in August 2011 Mike Brown published a list of 390 candidate objects, ranging from ""nearly certain"" to ""possible"" dwarf planets. Brown currently identifies eleven known objects – the five accepted by the IAU plus 2007 OR10, Quaoar, Sedna, Orcus, 2002 MS4 and Salacia – as ""virtually certain"", with another dozen highly likely. Stern states that there are more than a dozen known dwarf planets.However, only two of these bodies, Ceres and Pluto, have been observed in enough detail to demonstrate that they actually fit the IAU's definition. The IAU accepted Eris as a dwarf planet because it is more massive than Pluto. They subsequently decided that unnamed trans-Neptunian objects with an absolute magnitude brighter than +1 (and hence a diameter of ≥838 km assuming a geometric albedo of ≤1) are to be named under the assumption that they are dwarf planets. The only two such objects known at the time, Makemake and Haumea, went through this naming procedure and were declared to be dwarf planets. The question of whether other likely objects are dwarf planets has never been addressed by the IAU. The classification of bodies in other planetary systems with the characteristics of dwarf planets has not been addressed.